The goals of Group 2 were to reproduce and then produce variations on Petigura et. al. (2013) Figure 2, the binned planet occurrence rate f(P,Rp). We first binned the occurrence rates per planet provided by Group 1 in accordance with Petigura et. al. (2013) (Fig. \ref{pf2}), and then varied bin size to improve visibility of trends. After reproducing Petigura et. al. (2013) Figure 2 and producing the bin size variations, we repeated the plotting procedure for occurrence rate as a function of incident flux, rather than period.